Magnetospheric configuration for Parker-spiral IMF conditions: Results of a 3D AMR MHD simulation

被引：67

作者：

Gombosi, TI ^{[1
]}

DeZeeuw, DL ^{[1
]}

Groth, CPT ^{[1
]}

Powell, KG ^{[1
]}

机构：

[1] Univ Michigan, Ann Arbor, MI 48109 USA

来源：

SPACE WEATHER: PHYSICS AND APPLICATIONS | 2000年 / 26卷 / 01期

关键词：

D O I：

10.1016/S0273-1177(99)01040-6

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The global configuration and topology of the terrestrial magnetosphere for typical IMF conditions is simulated with a new 3D MHD model using adaptive mesh refinement (AMR), The paper briefly describes the main elements of the solution method and presents a steady-slate solution for nominal Parker-spiral IMF conditions, The simulated magnetic field topology in the magnetotail is in excellent agreement with the recent empirical model derived from four years of LMP 8 observations (Kaymaz and Siscoe, 1998). (C) 2000 COSPAR. Published by Elsevier Science Ltd.

引用

页码：139 / 149

页数：11

共 43 条

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